Vivanco Hector K, Trump Benjamin A, Brown Craig M, McQueen Tyrel M
Department of Chemistry, The Johns Hopkins University, Baltimore, Maryland 21218, USA.
Institute for Quantum Matter, Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, Maryland 21218, USA.
Phys Rev B. 2020 Dec;102(22). doi: 10.1103/PhysRevB.102.224411.
The Kitaev model is a rare example of an analytically solvable and physically instantiable Hamiltonian yielding a topological quantum spin liquid ground state. Here we report signatures of Kitaev spin liquid physics in the honeycomb magnet LiCoSbO, built of high-spin (Co) ions, in contrast to the more typical low-spin electron configurations in the presence of large spin-orbit coupling. Neutron powder diffraction measurements, heat capacity, and magnetization studies support the development of a long-range antiferromagnetic order space group of , below at . The magnetic entropy recovered between and 50 K is estimated to be , in good agreement with the value expected for systems close to a Kitaev quantum spin liquid state. The temperature-dependent magnetic order parameter demonstrates a value of 0.19(3), consistent with XY anisotropy and in-plane ordering, with Ising-like interactions between layers. Further, we observe a spin-flop-driven crossover to ferromagnetic order with space group of under an applied magnetic field of at . Magnetic structure analysis demonstrates these magnetic states are competing at finite applied magnetic fields even below the spin-flop transition. Both the compass model, a quantitative comparison of the specific heat of LiCoSbO, and related honeycomb cobaltates to the anisotropic Kitaev model further support proximity to a Kitaev spin liquid state. This material demonstrates the rich playground of high-spin systems for spin liquid candidates and complements known Ir- and Ru-based materials.
基泰耶夫模型是一个罕见的例子,它是一个可解析求解且可物理实现的哈密顿量,能产生拓扑量子自旋液体基态。在此,我们报告了在由高自旋(Co)离子构成的蜂窝状磁体LiCoSbO中基泰耶夫自旋液体物理的特征,这与在存在大自旋 - 轨道耦合时更典型的低自旋电子构型形成对比。中子粉末衍射测量、热容和磁化研究支持了在低于 时,在 空间群中长程反铁磁序的发展。在 和50 K之间恢复的磁熵估计为 ,这与接近基泰耶夫量子自旋液体状态的系统预期值非常吻合。温度依赖的磁序参量显示值为0.19(3),与XY各向异性和面内有序一致,层间存在类伊辛相互作用。此外,我们观察到在 时施加 的磁场下,自旋翻转驱动向具有 空间群的铁磁序的转变。磁结构分析表明,即使在自旋翻转转变以下的有限外加磁场中,这些磁态也相互竞争。 罗盘模型、LiCoSbO的比热与各向异性基泰耶夫模型的定量比较以及相关的蜂窝状钴酸盐都进一步支持了接近基泰耶夫自旋液体状态。这种材料展示了高自旋 系统作为自旋液体候选材料的丰富研究领域,并补充了已知的基于Ir和Ru的材料。